Search Publications

The Correlation of Outflow Kinematics with Star Formation Rate. VI. Gas Outflows in AGNs
DOI: 10.3847/1538-4357/abad97 Bibcode: 2020ApJ...901...66W

Rakshit, Suvendu; Woo, Jong-Hak; Son, Donghoon

We investigate the connection between ionized gas outflows and star formation activity using a large sample of type 1 and 2 active galactic nuclei (AGNs) with far-infrared detections or star formation rate (SFR) estimates. The strength of ionized gas outflows, measured by the velocity dispersion and velocity shift of the [O III] emission line, cle…

2020 The Astrophysical Journal
AKARI Herschel 22
The Drivers of Active Region Outflows into the Slow Solar Wind
DOI: 10.3847/1538-4357/ab8a4c Bibcode: 2020ApJ...894..144B

Golub, Leon; Winebarger, Amy R.; Warren, Harry P. +13 more

Plasma outflows from the edges of active regions have been suggested as a possible source of the slow solar wind. Spectroscopic measurements show that these outflows have an enhanced elemental composition, which is a distinct signature of the slow wind. Current spectroscopic observations, however, do not have sufficient spatial resolution to disti…

2020 The Astrophysical Journal
Hinode 22
The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. I. Survey Overview and First Results for Andromeda I
DOI: 10.3847/1538-4357/ab88a2 Bibcode: 2020ApJ...894..135S

Javadi, Atefeh; Saremi, Elham; van Loon, Jacco Th. +10 more

An optical monitoring survey in nearby dwarf galaxies was carried out with the 2.5 m Isaac Newton Telescope. Fifty-five dwarf galaxies and four isolated globular clusters in the Local Group were observed with the Wide Field Camera. The main aims of this survey are to identify the most evolved asymptotic giant branch (AGB) stars and red supergiants…

2020 The Astrophysical Journal
Gaia 21
A Chemo-dynamical Link between the Gjöll Stream and NGC 3201
DOI: 10.3847/1538-4357/ababa5 Bibcode: 2020ApJ...901...23H

Marshall, J. L.; Sneden, C.; Hansen, T. T. +4 more

Recent analysis of the second data release of Gaia has revealed a number of new stellar streams surrounding the Milky Way. It has been suggested that one of these streams, Gjöll, is associated with the globular cluster NGC 3201, but thus far the association has only been based on kinematics of the stream stars. In this work we identify five likely…

2020 The Astrophysical Journal
Gaia 21
Low-level Carbon Monoxide Line Polarization in Two Protoplanetary Disks: HD 142527 and IM Lup
DOI: 10.3847/1538-4357/abaef7 Bibcode: 2020ApJ...901...71S

Li, Zhi-Yun; Teague, Richard; Looney, Leslie W. +2 more

Magnetic fields are expected to play an important role in accretion processes for circumstellar disks. However, measuring the magnetic field morphology is difficult, especially when given that polarimetric (sub)millimeter continuum observations may not trace the fields in most disks. The Goldreich-Kylafis effect suggests that line polarization is …

2020 The Astrophysical Journal
Gaia 21
GeV γ-Ray Emission from M33 and Arp 299
DOI: 10.3847/1538-4357/aba043 Bibcode: 2020ApJ...901..158X

Liu, Ruo-Yu; Zhang, Hai-Ming; Wang, Xiang-Yu +1 more

Star-forming galaxies are huge reservoirs of cosmic rays (CRs) and these CRs convert a significant fraction of their energy into γ-rays by colliding with the interstellar medium (ISM). Several nearby star-forming galaxies have been detected in GeV-TeV γ-rays. It is also found that the γ-ray luminosities in 0.1-100 GeV correlate well with indicator…

2020 The Astrophysical Journal
Herschel 21
Angular Expansion of Nova Shells
DOI: 10.3847/1538-4357/ab76c5 Bibcode: 2020ApJ...892...60S

Guerrero, M. A.; Toalá, J. A.; Santamaría, E. +4 more

Nova shells can provide important information on their distance, their interactions with circumstellar and interstellar media, and the evolution in morphology of the ejecta. We have obtained narrowband images of a sample of five nova shells, namely DQ Her, FH Ser, T Aur, V476 Cyg, and V533 Her, with ages ranging from 50 to 130 yr. These images hav…

2020 The Astrophysical Journal
Gaia eHST 21
The First Extensive Spectroscopic Study of Young Stars in the North America and Pelican Nebulae
DOI: 10.3847/1538-4357/abba84 Bibcode: 2020ApJ...904..146F

Fang, Min; Herczeg, Gregory J.; Wang, Hongchi +5 more

We present a spectroscopic survey of over 3400 potential members in the North America and Pelican Nebulae (NAP) using several low-resolution (R ≈ 1300-2000) spectrographs: Palomar/Norris, WIYN/Hydra, Keck/DEep Imaging Multi-Object Spectrograph (DEIMOS), and the Multiple Mirror Telescope (MMT)/Hectospec. We identify 580 young stars as likely member…

2020 The Astrophysical Journal
Gaia 21
A New Likely Redback Millisecond Pulsar Binary with a Massive Neutron Star: 4FGL J2333.1-5527
DOI: 10.3847/1538-4357/ab77ba Bibcode: 2020ApJ...892...21S

Strader, Jay; Dage, Kristen C.; Chomiuk, Laura +7 more

We present the discovery of a likely new redback millisecond pulsar (MSP) binary associated with the Fermi γ-ray source 4FGL J2333.1-5527. Using optical photometric and spectroscopic observations from the Southern Astrophysical Research telescope, we identify a low-mass, main-sequence-like companion in a 6.9 hr, highly inclined orbit around a susp…

2020 The Astrophysical Journal
XMM-Newton 21
The Importance of Star Formation Intensity in Lyα Escape from Green Pea Galaxies and Lyman Break Galaxy Analogs
DOI: 10.3847/1538-4357/ab7895 Bibcode: 2020ApJ...893..134K

Malhotra, Sangeeta; Butler, Nathaniel R.; Yang, Huan +2 more

We have studied ultraviolet images of 40 Green Pea galaxies and 15 local Lyman Break Galaxy Analogs to understand the relation between Lyα photon escape and central UV photometric properties. We measured star-formation intensity (SFI; star formation rate per unit area) from the central 250 pc region ( ${S}_{250\mathrm{pc}}$ ) using Cosmic Origins …

2020 The Astrophysical Journal
eHST 21